Volume 42 Issue 11
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Li Rong, Wang Sen, Shi Huli. Thermal effect on inner-shield in main optical telescope of solar space telescope[J]. Infrared and Laser Engineering, 2013, 42(11): 2974-2978.
Citation: Li Rong, Wang Sen, Shi Huli. Thermal effect on inner-shield in main optical telescope of solar space telescope[J]. Infrared and Laser Engineering, 2013, 42(11): 2974-2978.

Thermal effect on inner-shield in main optical telescope of solar space telescope

  • Received Date: 2013-03-07
  • Rev Recd Date: 2013-04-09
  • Publish Date: 2013-11-25
  • The SST (Space Solar Telescope) is designed to obtain its diffraction limit quality with aperture over 1 m. It observes the sun with a small view field of 2.8'1.5' to obtain its high spatial resolution imaging of 0.1-0.15. SST observing the sun directly can receive huge heat flow more than 1 000 W that will lead to unacceptable thermal distortion of the optical components. The sunlight enters into the telescope, which is an intense source of both heat and stray light. Based on the special thermal effect and stray light in the solar telescope, a compatibility analysis of the thermal effect of inner-shield in SST was performed. The relationship between the thermal control design and scatting elimination plan on the inner-shield structures in SST was presented. The objective and method of the compatibility analysis were determined. With the thermal analysis software, the temperature fields were calculated for a series of heights of inner-shield structure. A design of the inner-shield structure was put forward in thermal control terms and the suggestion was put out synchronously, which restrained the inner-shield with the height less than 400 mm. The aims of the optimal design of the inner-shield structure of SST are reached. The thoughts and methods of the optimal analysis are also useful for similar optical telescopes designed for solar observation.
  • [1]
    [2] Stefan Dwnis, Pierre Coucke, Eric Gabriel, et al. Multi-application solar telescope: assembly, integration and testing[C]//SPIE, 2010, 7733: 773335.
    [3] Stefan Denis, Pierre Coucke, Eric Gabriel, et al. Optomechanical thermal design of the multi-application solar telescope for USO[C]//SPIE, 2008, 7012: 701235.
    [4]
    [5]
    [6] Thomas Rimmele, Stephen L Keil, Christoph Keller, et al. Technical challenges of the advanced technology solar telescope[C]//SPIE, 2003, 4837: 94-109.
    [7]
    [8] Suematsu Y, Katsukawa Y, Shimizu T, et al. Short telescope design of 1.5m aperture solar UV visible and IR telescope aboard solar-C[C]//SPIE, 2011, 8148: 81480D.
    [9] Meftah M, Irbah A. The space instrument SOOISM, a telescope to measure the solar diameter[C]//SPIE, 2011, 8146: 81460Z.
    [10]
    [11] Ester Antonucci, Marco Romoli, Daniele Gardiol, et al. Ultraviolet and visible-light coronagraphic iimager(UVCI) for HERSCHEL (Helium Resonance Scattering in Corona HELiosphere)[C]//SPIE, 2003, 4853: 162-171.
    [12]
    [13]
    [14] Wang S. Study on Thermal-Optical of Space Solar Telescope[M]. Beijing: National Astronomical Observatories, Chinese Academy of Sciences, 2005: 98-122.
    [15] Li Rong, Wang Sen. Thermal analysis of the baffle structure of the solar space telescope[J]. Science China: Physics, Mechanics and Astronomy, 2010, 53(9): 1755-1764.
    [16]
    [17]
    [18] Breault Robert P. Problems and techniques in stray radiation suppression[C]//SPIE, 1977, 107: 2-23.
    [19] Li Rong, Wang Sen, Shi Huli. Thermal effect on the vanes in the main optical telescope of the solar space telescope[J]. Infrared and Laser Engineering, 2013, 42(5): 1291-1297. (in Chinese)
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Thermal effect on inner-shield in main optical telescope of solar space telescope

  • 1. School of Mechanical Engineering,Hangzhou Dianzi University,Hangzhou 310018,China;
  • 2. National Astronomical Observatories,Chinese Academy of Sciences,Beijing 100012,China

Abstract: The SST (Space Solar Telescope) is designed to obtain its diffraction limit quality with aperture over 1 m. It observes the sun with a small view field of 2.8'1.5' to obtain its high spatial resolution imaging of 0.1-0.15. SST observing the sun directly can receive huge heat flow more than 1 000 W that will lead to unacceptable thermal distortion of the optical components. The sunlight enters into the telescope, which is an intense source of both heat and stray light. Based on the special thermal effect and stray light in the solar telescope, a compatibility analysis of the thermal effect of inner-shield in SST was performed. The relationship between the thermal control design and scatting elimination plan on the inner-shield structures in SST was presented. The objective and method of the compatibility analysis were determined. With the thermal analysis software, the temperature fields were calculated for a series of heights of inner-shield structure. A design of the inner-shield structure was put forward in thermal control terms and the suggestion was put out synchronously, which restrained the inner-shield with the height less than 400 mm. The aims of the optimal design of the inner-shield structure of SST are reached. The thoughts and methods of the optimal analysis are also useful for similar optical telescopes designed for solar observation.

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